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相关论文: Detection of Cyclotron Resonance Scattering Featur…

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We report comprehensive spectral and temporal properties of the Be/X-ray binary pulsar SMC X-2 using X-ray observations during the 2015 and 2022 outbursts. The pulse profile of the pulsar is unique and strongly luminosity dependent. It…

高能天体物理现象 · 物理学 2023-03-21 G. K. Jaisawal , G. Vasilopoulos , S. Naik , C. Maitra , C. Malacaria , B. Chhotaray , K. C. Gendreau , S. Guillot , M. Ng , A. Sanna

We present broadband X-ray observations of the High Mass X-ray Binary (HMXB) pulsar SMC X-2, using concurrent NuSTAR and NICER observations during its 2022 outburst. The source is found to be spinning with a period of 2.37281(3) s. We…

高能天体物理现象 · 物理学 2025-01-08 Mohammed Tobrej , Binay Rai , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

We report results of a spectral and timing analysis of the poorly studied transient X-ray pulsar 2S 1553-542 using data collected with the NuSTAR and Chandra observatories and the Fermi/GBM instrument during an outburst in 2015. Properties…

We report on the results of Swift and XMM-Newton observations of SMC X-2 during its last outburst in 2015 October, the first one since 2000. The source reached a very high luminosity ($L \sim 10^{38}$ erg s$^{-1}$), which allowed us to…

高能天体物理现象 · 物理学 2016-03-23 N. La Palombara , L. Sidoli , F. Pintore , P. Esposito , S. Mereghetti , A. Tiengo

We report the results of an analysis of data obtained with the INTEGRAL, Swift and RXTE observatories during the 2010 April and September outbursts of the X-ray pulsar RX J0440.9+4431. The temporal and spectral properties of the pulsar in a…

高能天体物理现象 · 物理学 2015-06-03 S. Tsygankov , R. Krivonos , A. Lutovinov

Cyclotron resonance scattering features or cyclotron absorption lines are unique features observed in the hard X-ray spectra of accretion powered X-ray pulsars with magnetic field of the order of 10$^{12}$ G. Detection of these features…

高能天体物理现象 · 物理学 2017-05-17 Gaurava K. Jaisawal , Sachindra Naik

We have monitored a Type II outburst of the Be/X-ray binary MXB 0656-072 in a series of pointed RXTE observations during October through December 2003. The source spectrum shows a cyclotron resonance scattering feature at 32.8 +/- 0.5 keV,…

We report the orbital X-ray variability of high mass X-ray binary (HMXB) GX301--2. GX301--2 undergone a spin up process in 2018--2020 with the period evolving from $\sim$ 685 s to 670 s. The energy resolved pulse-profiles of the pulsar in…

高能天体物理现象 · 物理学 2022-08-24 Y. Z. Ding , W. Wang , P. R. Epili , Q. Liu , M. Y. Ge , F. J. Lu , J. L. Qu , L. M. Song , S. Zhang , S. N. Zhang

We present spectral and timing analysis of NuSTAR observations of RX J0520.5$-$6932 in the 3-79 keV band collected during its outburst in January 2014. The target was observed on two epochs and we report the detection of a cyclotron…

We report results of a spectral and timing analysis of the X-ray pulsar XTE J1829-098 using data obtained with the NuSTAR observatory during an outburst in August 2018. A strong absorption feature was detected at the energy of…

高能天体物理现象 · 物理学 2018-10-17 Andrey E. Shtykovsky , Alexander A. Lutovinov , Sergey S. Tsygankov , Sergey V. Molkov

We report X-ray observations of the High Mass X-ray Binary (HMXB) pulsar 4U 1907+09. Spectral and Timing analysis of the source has been performed using NuSTAR observation. Timing analysis of the photon events revealed the coherent X-ray…

高能天体物理现象 · 物理学 2022-11-14 Mohammed Tobrej , Binay Rai , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

We report a time-resolved analysis of the accreting X-ray pulsar Cen X-3 using observations carried out by NuSTAR, which cover approximately two binary orbits in different intensity states. The pulse profile is relatively stable over the…

高能天体物理现象 · 物理学 2024-10-30 Qi Liu , Wei Wang , Andrea Santangelo , Lingda Kong , Long Ji , Lorenzo Ducci

IGR J0607.4+2205 is a transient Be X-ray binary discovered two decades ago. IGR J0607.4+2205 underwent an outburst in 2023 during which it was observed twice with \textit{NuSTAR}. The main goal of this work is to model the broadband X-ray…

高能天体物理现象 · 物理学 2024-02-28 Kinjal Roy , Rahul Sharma , Hemanth Manikantan , Biswajit Paul

The present paper reports on the RXTE observations of the binary X-ray pulsar 4U0115+63, covering an outburst in 1999 March-April with 44 pointings. The 3-30 keV PCA spectra and the 15-50 keV HEXTE spectra were analyzed jointly for the…

天体物理学 · 物理学 2008-11-26 Motoki Nakajima , Tatehiro Mihara , Kazuo Makishima , Hisako Niko

We present the results obtained from timing and spectral studies of the newly discovered accreting X-ray binary pulsar Swift J0243.6+6124 using a NuSTAR observation in 2017 October at a flux level of ~280 mCrab. Pulsations at 9.85423(5) s…

高能天体物理现象 · 物理学 2017-11-30 Gaurava K. Jaisawal , Sachindra Naik , J. Chenevez

OAO 1657-415 is an accreting X-ray pulsar with a high mass companion that has been observed by several telescopes over the years, in different orbital phases. Back in 1999, observations performed with Beppo-SAX lead to the detection of a…

高能天体物理现象 · 物理学 2022-03-08 Enzo A. Saavedra , Federico A. Fogantini , Jorge A. Combi , Federico García , Sylvain Chaty

The high-mass X-ray binary and accreting X-ray pulsar IGR J16393-4643 was observed by NuSTAR in the 3-79 keV energy band for a net exposure time of 50 ks. We present the results of this observation which enabled the discovery of a cyclotron…

We present the results of our spectral and timing analysis of the emission from the transient X-ray pulsar XTE J1946+274 based on the simultaneous NuSTAR and Swift/XRT observations in the broad energy range 0.3-79 keV carried out in June…

高能天体物理现象 · 物理学 2021-10-12 A. S. Gorban , S. V. Molkov , S. S. Tsygankov , A. A. Lutovinov

We report the time resolved spectroscopy result from two observations of Cen X-3, over one binary orbit with ASTROSAT and two binary orbit with NuSTAR. NuSTAR covered two intensity states where the light curve showed transition in count…

高能天体物理现象 · 物理学 2023-11-27 Pravat Dangal , Ranjeev Misra , Nand Kumar Chakradhari , Yashpal Bhulla

We study the timing and spectral properties of the X-ray pulsar 2S 1553--542 using the NuSTAR, and NICER during the outburst in January--February 2021. During the outburst, the spin period of the neutron star was 9.2822 s based on NuSTAR…

星系天体物理 · 物理学 2023-06-22 Manoj Mandal , Sabyasachi Pal
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